SDO HMI 2014-10-10 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.27 | 0.00 | 10.37 | 14.20 | 92.06 | 33.21 | 287.67 | 0.5573 | 72.4 | 63.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.53 | 10.92 | 101.75 | 42.90 | 279.42 | 0.6799 | -516.0 | -391.2 | |
| 0.00 | 0.88 | 0.00 | 0.59 | 11.30 | 101.53 | 42.68 | 280.00 | 0.6773 | -468.0 | -343.7 | |
| 0.00 | 1.58 | 0.00 | 1.06 | 11.04 | 101.40 | 42.55 | 279.62 | 0.6755 | -721.0 | -673.6 | |
| 0.00 | 1.14 | 0.00 | 0.73 | 11.90 | 98.70 | 39.85 | 281.19 | 0.6415 | -701.0 | -601.3 | |
| 0.00 | 0.96 | 0.00 | 0.62 | 12.45 | 98.56 | 39.71 | 282.07 | 0.6403 | -624.0 | -571.9 | |
| 0.00 | 1.66 | 0.00 | 1.02 | 10.70 | 95.35 | 36.50 | 279.66 | 0.5952 | -724.0 | -571.0 | |
| 0.00 | 0.53 | 0.00 | 0.32 | 11.97 | 94.90 | 36.05 | 281.86 | 0.5905 | -302.0 | -375.3 | |
| 0.00 | 0.88 | 0.00 | 0.52 | 13.95 | 91.12 | 32.27 | 286.28 | 0.5419 | 551.0 | 420.3 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 14.83 | 87.87 | 29.02 | 289.20 | 0.4986 | 680.0 | 518.2 | |
| 0.00 | 1.93 | 0.00 | 1.09 | 15.45 | 87.01 | 28.16 | 290.85 | 0.4887 | 802.0 | 696.2 | |
| 0.00 | 2.19 | 0.00 | 1.24 | 19.83 | 85.33 | 26.48 | 300.44 | 0.4885 | 695.0 | 574.5 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 16.98 | 84.33 | 25.48 | 295.62 | 0.4583 | 786.0 | 679.1 | |
| 0.00 | 1.49 | 0.00 | 0.83 | 16.71 | 84.26 | 25.41 | 295.12 | 0.4558 | 729.0 | 567.5 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 16.65 | 82.77 | 23.92 | 296.13 | 0.4345 | 826.0 | 659.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |